CWWDL 14199

0.14 UTI

0.52

C_N

0.81

C_dens

1.0

C_C3

0.0

C_lit

0.29

C_dup

C3 classification AA

Number of members (P>50%) 55

Radius (P>50% members) 9.0 [arcmin]

C_N 0.52 Moderately populated
C_dens 0.81 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.29 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 14199 is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14199 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	268.605	-23.086	0.711	0.08	-2.611	0.136
Chi et al.	2023	268.618	-23.089	0.719	0.091	-2.6	6.744

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Chi et al.	2023	–	–	–	14	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1761	90.9	268.6	-23.09	0.71	0.08	-2.61	-5.4	0.06
UFMG 72	70.9	268.53	-23.13	0.71	0.08	-2.61	-10.55	0.48

💡 Note: The % column shows the percentage of members that CWWDL 14199 shares with each listed object.

Visualization

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